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Searching Rudolf Steiner Lectures by GA number (GA0323)
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    Query was: three
  

Here are the matching lines in their respective documents. Select one of the highlighted words in the matching lines below to jump to that point in the document.

  • Title: Astronomy Course: Lecture I
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    • three men could scarcely understand one another. The one who
    • geometrical conception of three-dimensional space; — to
  • Title: Astronomy Course: Lecture II
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    • his cosmic system upon three axioms. The first is that the
    • external phenomena surrounding man from three different
    • first in quite a popular, even elementary way how these three
    • that there exists a certain connection between this threefold
    • must have a connection with the three-fold being of man.
    • three members of the threefold man. When we bring this into
    • human form — the threefold being of man. Thus do the
  • Title: Astronomy Course: Lecture III
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    • on this account was he able to draw up his three famous Laws
    • For modern Astronomy the three famous Laws of Kepler are
  • Title: Astronomy Course: Lecture V
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    • the three-foldness of the being of man, recognized as a
    • three forms of processes all that is functional in man is
    • organism is derivable from these three.
    • learning to understand man in this threefold aspect we must
    • observe that he is connected with the outer world in a three
    • what is manifested therefore at the two poles of threefold
    • threefold human nature, organized now in one way, now in
  • Title: Astronomy Course: Lecture VI
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    • the Earth today are such that we have the three types; the
  • Title: Astronomy Course: Lecture VII
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    • which is characterized by three rigid directions at right
    • reality, to justify our setting up the three coordinate axes
  • Title: Astronomy Course: Lecture VIII
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    • mood of soul. We spoke of his three Laws — a work of
    • harmony. He felt has three planetary Laws as a last
  • Title: Astronomy Course: Lecture X
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    • Cassini curve. We know that this curve has three, or, if you
    • create three-dimensional forms then I should obtain bodies
  • Title: Astronomy Course: Lecture XII
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    • three formative principles
    • of three Suns instead of one. So they distinguished three
    • Modern Astronomy too has its three Suns. There is the Sun
    • distinguishes three: the real Sun and two imagined ones. It
    • needs the three, for what is calculated to begin with does
    • remain behind. Thus if we study the three kingdoms quite
  • Title: Astronomy Course: Lecture XIII
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    • the same magnitude for all three planets. Nay more, it is the
  • Title: Astronomy Course: Lecture XIV
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    • contemporaries: I look at three successive positions of what
    • three, and we shall say to ourselves: Something in us is the
    • outcome of the substantialities of these three spheres. Here
    • mathematician's bugbear — the “problem of three
    • connected with the problem of three bodies, Earth, Sun and
    • centre-of-gravity of the three bodies — Sun, Moon and
    • of three bodies', yet it is solved, namely in Man. When man
    • point-of-intersection of the three influences. It is
  • Title: Astronomy Course: Lecture XV
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    • Geometry, that is to say, within a rigid three-dimensional
    • Three*, we get into formidable difficulties in spatial
    • goes with it in the organization three independent systems
    • this question: How are the three members of the three-fold
    • be only pictorial to begin with — of how the three members of
    • threefold system thus presented we have the key to the
    • the Cassini curve, we showed that it has three essential
    • than three dimensional space affords. Thinking in this way,
    • ordinary space, conceived in its three dimension, but with a
    • Suppose I form the thought of ordinary, three-dimensional,
    • and mental presentation of it — three-dimensional space with
    • debt. Likewise I cannot only make the three dimensions to
    • think only two dimensions instead of three, but that is not
    • source that can no longer be there in my three-dimensional
    • ordinary straight line drawn into three-dimensional space. It
    • successive vanishing of three dimensions. Now let us suppose
    • quite outside three-dimensional space. What then shall we
    • to what is quite outside three-dimensional space.
    • what is outside it three-dimensional space altogether. We can
    • deleted", but only to what deletes all three of them, z, y,
    • Maximum number of matches per file exceeded.
  • Title: Astronomy Course: Lecture XVII
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    • of today uses three Suns in its calculations: the real Sun,



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